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- 23:33, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:31, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:30, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:27, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:25, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:23, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:21, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:20, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:17, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:12, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:09, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:07, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:04, 10 September 2013 (diff | hist) N File:Fig6.jpg (Plasma density (color scale) around the descending intrusion (black disk) at three different times. The red curve along the right of each panel shows the density along the flux tube outlined in white.) (top)
- 23:01, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 23:00, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 22:57, 10 September 2013 (diff | hist) N File:Fig5.jpg (Flow Mach number (top) and density (bottom) along a flux tube plotted as a thick black curve. The flow enters with a specified speed (red). It shocks onto the transonic curve (blue) to pass the point of maximum constriction (z=0). It then shocks onto ) (top)
- 22:49, 10 September 2013 (diff | hist) N File:Fig3.jpg (Flux tubes in layer surrounding a current sheet (thick red curve) deformed by a descending intrusion (black disk). One flux tube is outlined in blue and its cross sectional area is shown as a blue curve along the left edge.) (top)
- 22:47, 10 September 2013 (diff | hist) Peristaltic Shocks: a model
- 22:45, 10 September 2013 (diff | hist) N Peristaltic Shocks: a model (Created page with "<b>Background</b> In standard models of magnetic reconnection virtually all of the released energy remains on those field lines that have reconnected. The small amount of magne...")